Transparency of the Inner Heliosphere to the Interstellar Dust Stream During Solar Maximum: Ulysses Measurements and Modelling

Details Transparency of the Inner Heliosphere to the Interstellar Dust Stream During Solar Maximum: Ulysses Measurements and Modelling Transparency of the Inner Heliosphere to the Interstellar Dust Stream During Solar Maximum: Ulysses Measurements and Modelling

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1306l&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1306

Physics

Scientific paper

The Ulysses dust detector has detected an increased flux of interstellar
dust grains since early 2000. This elevated flux is observed up to the
most recent data end-2002. Only relatively small dust grains with high
charge to mass ratios can explain the observations.

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